Magnetized Quark Matter Grows Stiffer When Isospin Imbalance Enters the Equation
A new one-loop hard-dense-loop calculation reveals that cold quark matter under ultra-strong magnetic fields becomes paramagnetic and develops strongly anisotropic ...
A new one-loop hard-dense-loop calculation reveals that cold quark matter under ultra-strong magnetic fields becomes paramagnetic and develops strongly anisotropic ...
A new theoretical analysis shows that a maximally charged thin shell in Einstein gravity coupled to Born–Infeld electrodynamics can be ...
A lattice-constrained effective model reveals sharp peaks in specific heat and a rapid stiffening of the isentropic bulk modulus as ...
The Einstein Probe mission has captured a previously hidden, minutes-long soft X-ray phase accompanying a short gamma-ray burst, providing direct ...
A holographic string-theory model of dense quark matter predicts stable compact stars with quark cores reaching masses of up to ...
A hybrid Padé semi-cosmographic framework combining DESI DR2 baryon acoustic oscillation data with mock 21 cm intensity-mapping forecasts tightly constrains ...
A new review explains why turbulence is the central unsolved challenge in simulating neutron star mergers and how relativistic large-eddy ...
A comprehensive review shows how ab initio simulations of warm dense matter are decoding the interiors, evolution, and magnetic fields ...
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© 2025 Scienmag - Science Magazine